at_data: Documentation on the atomic reference data
Package: nebular
References
The atomic data for hydrogen were taken from Brocklehurst (1970, 1971); in particular, we adopt an empirical formula from Aller (1984) for the H-beta line emissivity. The other atomic data were taken from the following references:
Table 1. References for Recent Atomic Data
-----------------------------------------
Ion Parameters Source
-----------------------------------------
C I Energy levels:
5 levels B60
6th level NS84
Trans. probabilities FS85
Coll. strengths:
2-1, 3-1, 3-2 JBK87
all other PA76
-----------------------------------------
C II Energy levels:
2nd level KS86
6,7,8th levels NS81
all other WL95
Trans. probabilities:
2-1, 4-3, 5-3, 5-4 NS81
all other F94
Coll. strengths BP92
_________________________________________
C III Energy levels BK92
Trans. probabilities:
4-2 G83
3-2 NS78
all other WFD96
Coll. strengths BBDK85
_________________________________________
N I Energy levels:
2 & 3 levels B60
4 & 5 levels KS86
6,7,8th levels F75
Trans. probabilities:
5-4 KS86
all other WFD96
Coll. strengths:
4,5th levels PA76
all other DMR76
_________________________________________
N II Energy levels:
5 levels B60
6-2 WL95
Trans. probabilities WFD96
Coll. strengths LB94
_________________________________________
N III Energy levels:
5 levels BFJ95
6,7,8th levels BP92
Trans. probabilities:
2-1 F83
all other BFJ95
Coll. strengths BP92
_________________________________________
N IV Energy levels M49
Trans. probabilities:
3-2 NS79
4-2 G83
all other WFD96
Coll. strengths RBHB93
_________________________________________
O I Energy levels B60
Trans. probabilities WFD96
Coll. strengths BK95
_________________________________________
O II Energy levels:
2 & 3 levels B60
4 & 5 levels KS86
6,7,8th levels F75
Trans. probabilities WFD96
Coll. strengths:
3-2, 5-4 P76
all other MB93
_________________________________________
O III Energy levels:
5 levels B60
6-2 M85
Trans. probabilities WFD96
Coll. strengths LB94
_________________________________________
O IV Energy levels:
5 levels BJB96
6,7,8th levels BP92
Trans. probabilities:
2-1 KS86
5-4 WL95
all other BJB96
Coll. strengths BP92
_________________________________________
O V Energy levels:
2,4,5th levels BJ68
3rd level B80
Trans. probabilities:
3-1, 5-1 H80
all other NS79
Coll. strengths BBDK85
_________________________________________
Ne II Energy levels E83
Trans. probabilities:
2-1 BBB06
Coll. strengths GMB01
_________________________________________
Ne III Energy levels B60
Trans. probabilities:
3-1, 4-3, 5-1 M83
all other KS86
Coll. strengths BZ94
_________________________________________
Ne IV Energy levels M71
Trans. probabilities:
5 levels BBZ89
all other BK88
Coll. strengths G81
_________________________________________
Ne V Energy values:
5 levels B60
6-2 M83
Trans. probabilities:
6-2, 6-3 KS86
6-4 BD93
Coll. strengths LN94
_________________________________________
Ne VI Energy levels:
2nd level KS86
all others MVGK95
Trans. probabilities:
2-1 KS86
all other MVGK95
Coll. strengths ZGP94
_________________________________________
Na IV Energy levels B60
Trans. probabilities:
3-1, 4-3, 5-1 M83
all other KS86
Coll. strengths BZ94
_________________________________________
Na VI Energy levels B60
Trans. probabilities:
3-1, 4-1, 5-3 NR79
all other KS86
Coll. strengths LB94
_________________________________________
Mg V Energy levels B60
Trans. probabilities:
3-1, 4-3, 5-1 M83
all other KS86
Coll. strengths BZ94
_________________________________________
Mg VII Energy levels:
5 levels B60
6th level BD95
Trans. probabilities BD95
Coll. strengths LB94
_________________________________________
Al II Energy levels MZ79
Trans. probabilities:
3-1 JSP86
3-2, 4th levels HK87
5-1 VVF96
5-2, 5-3, 5-4 KS86
Coll. strengths:
3-2, 4-2, 4-3 KHAF92
5-1 TBK85
all other TBK84
_________________________________________
Si II Energy levels:
5 levels DKH91
6,7th levels BL93
8th level N77
Trans. probabilities:
3-2, 4-2, 5-2 CSB93
6-1, 6-2, 7-2 BL93
8-1, 8-2 L94
all other N77
Coll. strengths DK91
_________________________________________
Si III Energy levels WL95
Trans. probabilities:
3-1 OKH88
4-1, 4-2 M83
5-1 FW90
all other KS86
Coll. strengths DK94
_________________________________________
S II Energy levels:
5 levels B60
6,7 8th levels VVF96
Trans. probabilities:
6-1, 7-1, 8-1 VVF96
all other KHOC93
Coll. strengths RBS96
_________________________________________
S III Energy levels B60
Trans. probabilities:
3-1, 4-1, 5-3, 5-4 MZ82b
6-2, 6-3 HSC95
6-4 LL93
all other KS86
Coll. strengths GMZ95
_________________________________________
S IV Energy levels BDF80
Trans. probabilities:
2-1 JKD86
3,4,5th levels DHKD82
6-1, 6-2, 7-2
8-1, 8-2 VVF96
Coll. strengths DHKD82
_________________________________________
Cl III Energy levels B60
Trans. probabilities:
4-3 M83
all other KS86
Coll. strengths BZ89
_________________________________________
Cl IV Energy levels:
5 levels B60
6th level H85
Trans. probabilities:
3-1, 4-1, 5-3 MZ82b
6-2, 6-3 EM84
all other KS86
Coll. strengths GMZ95
_________________________________________
Ar II Energy levels BBB06
Trans. probabilities:
2-1 BBB06
Coll. strengths PB95
_________________________________________
Ar III Energy levels B60
Trans. probabilities:
3-1, 4-3, 5-1 M83
all other KS86
Coll. strengths GMZ95
_________________________________________
Ar IV Energy levels B60
Trans. probabilities:
4-3 MZ82a
all other KS86
Coll. strengths ZBL87
_________________________________________
Ar V Energy levels
5 levels B60
6th level H85
Trans. probabilities:
3-1, 4-1, 5-3 MZ82b
6th level LL93
all other KS86
Coll. strengths GMZ95
_________________________________________
K IV Energy levels B60
Trans. probabilities:
3-1, 4-3, 5-1 M83
all other KS86
Coll. strengths GMZ95
_________________________________________
K V Energy levels B60
Trans. probabilities:
4-3 M83
all other KS86
Coll. strengths BZL88
_________________________________________
Ca V Energy levels B60
Trans. probabilities:
3-1, 4-3, 5-1 M83
all other KS86
Coll. strengths GMZ95
_________________________________________
LITERATURE CITED
Aller, 1984, "Physics of Thermal Gaseous Nebulae"
(Dordrecht:D. Reidel)
Prevot, Lequeux, Maurice, Prevot & Rocca-Volmerange, 1984, A&A, 132, 389
REFERENCES TO ATOMIC DATA:
(BBB06) Badnell, et al. 2006, in IAUS 234, 211
(BBZ89) Becker, Butler & Zeippen 1989, A&A, 221, 375
(BL93) Bergeson & Lawler 1993, ApJ, 414, L137
(BBDK85) Berrington, Burke, Dufton & Kingston 1985, ADNDT, 33, 195
(BDF80) Bhatia, Doschek & Feldman 1980, A&A, 86, 32
(BD93) Bhatia & Doschek 1993, ADNDT, 55, 315
(BD95) Bhatia & Doschek 1995, ADNDT, 60, 145
(BK88) Bhatia & Kastner 1988, ApJ, 332, 1063
(BK92) Bhatia & Kastner 1992, ApJ, 408, 744
(BK95) Bhatia & Kastner 1995, ApJS, 96, 325
(BP92) Blum & Pradhan 1992, ApJS, 80 425
(BJ68) Bockasten & Johanssen 1968, Arkiv Fysik, 38, 563
(B60) Bowen, 1960 ApJ, 132, 1
(BFJ95) Brage, Froese-Fischer & Judge 1995, ApJ, 445, 457
(BJB96) Brage, Judge & Brekke 1996, ApJ 464, 1030
(BR70) Brocklehurst 1970, MNRAS, 148, 417
(BR71) Brocklehurst 1971, MNRAS, 153, 471
(B80) Brown 1980, A&A, 88, 273
(BZ89) Butler & Zeippen 1989, A&A, 208, 337
(BZ94) Butler & Zeippen 1994, A&AS, 108, 1
(BZL88) Butler, Zeippen & Le Bourlot, 1988, A&A, 203, 189
(CSB93) Calamai, Smith & Bergeson 1993, ApJ, 415, L59
(DMR76) Dopita, Mason & Robb 1976, ApJ, 207, 102
(DHKD82) Dufton, Hibbert, Kingston & Doschek 1982, ApJ, 257, 338
(DK91) Dufton & Kingston 1991, MNRAS, 248, 827
(DKH91) Dufton, Keenan, Hibbert, Stafford, Byrne & Agnew 1991, MNRAS, 253, 474
(DK94) Dufton & Kingston 1994, ADNDT, 57, 273
(E83) Edlen 1983, PhyS, 28, 51
(EM84) Ellis & Martinson 1984, Phys. Scr., 30, 255
(F75) Fawcett 1975, ADNDT, 16, 135
(F83) Froese-Fischer 1983, J. Phys. B, 16, 157
(FS85) Froese-Fischer & Saha, 1985, Phys. Scr., 32, 181
(F94) Froese-Fischer 1994, Phys. Scr., 49, 323
(FW90) Fuhr & Wiese 1990, CRC, 71st Edition
(GMZ95) Galavis, Mendoza & Zeippen 1995, A&A Supp., 111, 347
(G81) Giles 1981, MNRAS, 195, 5P
(G83) Glass 1983, Astrophy. Space Sci., 92, 307
(GMB01) Griffin, Mitnik, & Badnell 2001, JPhB, 34, 4401
(HSC95) Heise Smith & Calamai, 1995, ApJ, 451, L41
(G80) Hibbert 1980, J Phys B, 13, 1721
(HK87) Hibbert & Keenan, 1987, J. Phys. B, 20, 4693
(H85) Huang 1985, ADNDT, 32, 503
(JKD86) Johnson, Kingston & Dufton 1986, MNRAS, 220, 155
(JSP86) Johnson, Smith & Parkinson 1986, ApJ, 308, 1013
(JBK87) Johnson, Burke & Kingston 1987, J Phys B, 20, 2553
(KS86) Kaufman & Sugar 1986, JPCRD, 15, 321
(KHAF92) Keenan, Harra, Agarwal & Feibelman 1992, ApJ, 385, 375
(KHOC93) Keenan, Hibbert Ojha & Caylon 1993, Phys. Scr., 48, 129
(LL93) LaJohn & Luke 1993, Phys. Scr., 47, 542
(L94) Lanzafame, 1994 A&A, 287, 972
(LB94) Lennon & Burke 1994, A&AS, 103, 273
(MZ79) Martin & Zalubas 1979, JPCRD, 8, 3
(MB93) McLaughlin & Bell 1993, ApJ, 408, 753
(MZ82) Mendoza & Zeippen 1982, MNRAS, 198,127
(MZ82) Mendoza & Zeippen 1982, MNRAS, 199, 1025
(M83) Mendoza 1983, "Planetary Nebulae", 143
(MVGK95) Merkelis, Vilkas, Gaigalas & Kisielius 1995, Phys. Scr., 51, 233
(M49) Moore 1949, NBS Circ., 467
(M71) Moore 1971, "Atomic Energy Levels", Vol. 1
(M85) Moore 1985, "Selected Tables of Atomic Spectra"
(M77) Nussbaumer 1977, A&A, 58, 291
(NR79) Nussbaumer & Rusca 1979, A&A, 72, 129
(NS78) Nussbaumer & Storey 1978, A&A, 64, 139
(NS79) Nussbaumer & Storey 1979, A&A, 74, 244
(NS81) Nussbaumer & Storey 1981, A&A, 96, 91
(NS84) Nussbaumer & Storey 1984, A&A, 140, 383
(OKH88) Ojha, Keenan & Hibbert 1988, JPhys. B, 21, L395
(PA76) Pequignot & Aldrovandi 1976, A&A, 50, 141
(P76) Pradhan 1976, MNRAS, 177, 31
(PB95) Pelan & Berrington 1995, A&AS, 110, 209
(RBHB93) Ramsbotton, Berrington, Hibbert & Bell 1993, Phys Scr., 50,
(RBS96) Ramsbottom, Bell & Stafford 1996, ADNDT, 63, 57
(Sh94) Shirai, Sugar, & Musgrove 1999, private comm.
(SMZ84) Smith, Magnusson & Zetterberg, 1984, ApJ, 277, L79
(TBK84) Tayal, Burke & Kingston 1984, J Phys B, 17, 3847
(TBK85) Tayal, Burke & Kingston 1985, J Phys B, 18, 4321
(VVF96) Verner D.A., Verner E.M. & Ferland 1996, ADNDT, 64, 1
(WFD96) Wiese, Fuhr & Deters 1996, JPCRD, Monograph 7
(WL95) Williams & Livio 1995, Proc. of STScI No. 8, 24
(ZBL87) Zeippen, Butler & Le Bourlot 1987, A&A, 188, 251
(ZGP94) Zhang, Graziani & Pradhan 1994, A&A, 283, 319
See also
Type "help nebular opt=sys" for a general description of the tasks in the `nebular' package.